Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  HD108090  ·  NGC 4395
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NGC4395, Revised, Vincent Goetz
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NGC4395, Revised

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NGC4395, Revised, Vincent Goetz
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NGC4395, Revised

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Description

NGC 4395 is a nearby low surface brightnessspiral galaxy located about 14 million light-years (or 4.3 Mpc) from Earth in the constellation Canes Venatici.  The nucleus of NGC 4395 is active and the galaxy is classified as a Seyfert Type I known for its very low-mass supermassive black hole.Physical characteristicsNGC 4395 has a halo that is about 8 in diameter. It has several patches of greater brightness running northwest to southeast. The one furthest southeast is the brightest. Three of the patches have their own NGC numbers: 4401, 4400, and 4399 running east to west.The galaxy is highly unusual for Seyfert galaxies, because it does not have a bulge and is considered to be a dwarf galaxy.[5]Observational historyNGC 4395 was imaged and classified as a "spiral nebula" in a 1920 paper by astronomerFrancis G. Pease.   Now, it is known to be a galaxy distinct from the Milky Way (see Great Debate). Along with several other nearby galaxies, resolved stars in NGC 4395 were used to measure the expansion rate of the Universe by Allan Sandage and Gustav Andreas Tammann in their 1974 paper.   More recently, NGC 4395 was discovered to contain a very low-luminosity active galactic nucleus.  Since then, its nucleus has been the subject of several academic papers and attempts to measure the mass of its central black hole.

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NGC4395, Revised, Vincent Goetz